Sedimentary Record of Impact Events in Spain
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Terrestrial Impact Structures Provide the Only Ground Truth Against Which Computational and Experimental Results Can Be Com Pared
Ann. Rev. Earth Planet. Sci. 1987. 15:245-70 Copyright([;; /987 by Annual Reviews Inc. All rights reserved TERRESTRIAL IMI!ACT STRUCTURES ··- Richard A. F. Grieve Geophysics Division, Geological Survey of Canada, Ottawa, Ontario KIA OY3, Canada INTRODUCTION Impact structures are the dominant landform on planets that have retained portions of their earliest crust. The present surface of the Earth, however, has comparatively few recognized impact structures. This is due to its relative youthfulness and the dynamic nature of the terrestrial geosphere, both of which serve to obscure and remove the impact record. Although not generally viewed as an important terrestrial (as opposed to planetary) geologic process, the role of impact in Earth evolution is now receiving mounting consideration. For example, large-scale impact events may hav~~ been responsible for such phenomena as the formation of the Earth's moon and certain mass extinctions in the biologic record. The importance of the terrestrial impact record is greater than the relatively small number of known structures would indicate. Impact is a highly transient, high-energy event. It is inherently difficult to study through experimentation because of the problem of scale. In addition, sophisticated finite-element code calculations of impact cratering are gen erally limited to relatively early-time phenomena as a result of high com putational costs. Terrestrial impact structures provide the only ground truth against which computational and experimental results can be com pared. These structures provide information on aspects of the third dimen sion, the pre- and postimpact distribution of target lithologies, and the nature of the lithologic and mineralogic changes produced by the passage of a shock wave. -
Evidence from the Northwestern Venezuelan Andes for Extraterrestrial Impact: the Black Mat Enigma
Geomorphology 116 (2010) 48–57 Contents lists available at ScienceDirect Geomorphology journal homepage: www.elsevier.com/locate/geomorph Evidence from the northwestern Venezuelan Andes for extraterrestrial impact: The black mat enigma W.C. Mahaney a,⁎, V. Kalm b, D.H. Krinsley c, P. Tricart d, S. Schwartz d, J. Dohm e,f, K.J. Kim g, B. Kapran a, M.W. Milner a, R. Beukens h, S. Boccia i, R.G.V. Hancock j, K.M. Hart k, B. Kelleher k a Quaternary Surveys, 26 Thornhill Ave., Thornhill, Ontario, Canada L4J 1J4 b Institute of Ecology & Earth Sciences, Tartu University, Tartu, EE51014, Estonia c Institute of Geological Sciences, University of Oregon, Eugene, Oregon, 97403-1272, USA d Laboratoire de Geodynamique des Chaînes Alpines, University of Grenoble, Observatoire des Sciences de l'Univers, 38041, Grenoble, France e Department of Hydrology and Water Resources, University of Arizona, Tucson, Az., 85721, USA f The Museum, The University of Tokyo, Tokyo, 113-0033, Japan g Geological Research Division (Prospective Geoscience Research Department), Korea Institute of Geoscience and Mineral Resources (KIGAM), 92 Gwahang-no, Yuseong-gu, Daejeon 305-350, Republic of Korea h IsoTrace Lab, Dept of Physics, University of Toronto, Toronto, Ontario, Canada M5S 1A7 i Department of Materials Science, University of Toronto, Toronto, Ontario, Canada M5S 3E4 j Department of Medical Physics and Applied Radiation Sciences and Department of Anthropology, McMaster University, Hamilton, Ontario, Canada L8S 4K1 k School of Chemical Sciences, Dublin City University, Ballymun Road, Glasnevin, Dublin 9, Ireland article info abstract Article history: A carbon-rich black layer encrusted on a sandy pebbly bed of outwash in the northern Venezuelan Andes, Received 11 January 2009 previously considered the result of an alpine grass fire, is now recognized as a ‘black mat’ candidate correlative Received in revised form 9 October 2009 with Clovis Age sites in North America, falling within the range of ‘black mat’ dated sites (~12.9 ka cal BP). -
A Study of the Brushy Creek Feature, Saint Helena Parish, Louisiana Andrew Schedl
Open-File Series No. 18-01 Fall 2018 A Study of the Brushy Creek Feature, Saint Helena Parish, Louisiana Andrew Schedl Abstract This study was unable to determine the origin of the Brushy Creek feature. New¯ thin sections were made and new and old thin sections were examined using the opti- cal and scanning electron microscope (SEM). Powdered samples from the center of Brushy Creek were examined using X-ray diffraction (XRD). In sample 16SHPA, a half dozen new grains with probable planar deformation features (PDF) were found with orientations of {1012} and {1011}. Preliminary SEM studies of zircons showed no evidence for PDFs or reidite. Only one grain from the center of Brushy Creek structure showed possible rectangular fracture. XRD analysis found no evidence for high-pressure forms of quartz, coesite and stishovite. Suggestions for further study are included. Introduction North-south oriented ridges and ravines dominate the landscape in this part of Louisiana. The Brushy Creek is a “noticeable circular hole” in the ridge/ravine topography (Heinrich, 2003). The feature is about 2 kilometers in diameter and has a relief of 15 meters and Brushy Creek breeches the southeast rim of this feature. Exposed in the rim is the poorly lithified and highly fractured Pliocene Citronelle Formation. Near the Brushy Creek feature, the Citronelle formation consists of cross-bedded, massive, poorly sorted fine to coarse sand 9-12 meters thick underlain by 6 meters of laminated clay and silt. The Kentwood Brick and Tile Company has drilled the center of the feature and have found that the laminated clay and silt is absent. -
Impact Cratering
6 Impact cratering The dominant surface features of the Moon are approximately circular depressions, which may be designated by the general term craters … Solution of the origin of the lunar craters is fundamental to the unravel- ing of the history of the Moon and may shed much light on the history of the terrestrial planets as well. E. M. Shoemaker (1962) Impact craters are the dominant landform on the surface of the Moon, Mercury, and many satellites of the giant planets in the outer Solar System. The southern hemisphere of Mars is heavily affected by impact cratering. From a planetary perspective, the rarity or absence of impact craters on a planet’s surface is the exceptional state, one that needs further explanation, such as on the Earth, Io, or Europa. The process of impact cratering has touched every aspect of planetary evolution, from planetary accretion out of dust or planetesimals, to the course of biological evolution. The importance of impact cratering has been recognized only recently. E. M. Shoemaker (1928–1997), a geologist, was one of the irst to recognize the importance of this process and a major contributor to its elucidation. A few older geologists still resist the notion that important changes in the Earth’s structure and history are the consequences of extraterres- trial impact events. The decades of lunar and planetary exploration since 1970 have, how- ever, brought a new perspective into view, one in which it is clear that high-velocity impacts have, at one time or another, affected nearly every atom that is part of our planetary system. -
COMUNICAR 47: 281; Number of Research Works Accepted: 10
© COMUNICAR, 47, XXIV MEDIA EDUCATION RESEARCH JOURNAL REVISTA CIENTÍFICA DE COMUNICACIÓN Y EDUCACIÓN ISSN: 1134-3478 / e-ISSN: 1988-3293 n. 47, vol. XXIV (2016-2), 2nd Quarter, April, 1st 2016 INDEXED INTERNATIONAL RESEARCH JOURNAL INTERNATIONAL DATABASES LIBRARY CATALOGUES • JOURNAL CITATION REPORTS (JCR) (Thomson Reuters)® •WORLDCAT • SOCIAL SCIENCES CITATION INDEX / SOCIAL SCISEARCH (Thomson Reuters) • REBIUN/CRUE •SCOPUS® • SUMARIS (CBUC) • ERIH+ (European Science Foundation) • NEW-JOUR • FRANCIS (Centre National de la Recherche Scientifique de Francia) • ELEKTRONISCHE ZEITSCHRIFTENBIBLIOTHEK (Electronic Journals Library) • SOCIOLOGICAL ABSTRACTS (ProQuest-CSA) • THE COLORADO ALLIANCE OF RESEARCH LIBRARIES • COMMUNICATION & MASS MEDIA COMPLETE • INTUTE (University of Manchester) • ERA (Educational Research Abstract) •ELECTRONICS RESOURCES HKU LIBRARIES (Hong Kong University, HKU) • IBZ (Internat. Bibliography of Periodical Literature in the Social Sciences) • BIBLIOTECA DIGITAL (University of Belgrano) • IBR (International Bibliography of Book Reviews in the Social Sciences) BIBLIOGRAPHICAL DATABASES •SOCIAL SERVICES ABSTRACTS • DIALNET (Alertas de Literatura Científica Hispana) • ACADEMIC SEARCH COMPLETE (EBSCO) • PSICODOC • MLA (Modern International Bibliography) • REDINED (Ministerio de Educación de Spain) • COMMUNICATION ABSTRACTS (EBSCO) • CEDAL (Instituto Latinoamericano de Comunicación Educativa: ILCE) • EDUCATION INDEX/Abstracts, OmniFile Full Text Megs/Select (Wilson) • OEI (Centro de Recursos de la Organización de Estados -
Multiple Fluvial Reworking of Impact Ejecta—A Case Study from the Ries Crater, Southern Germany
Multiple fluvial reworking of impact ejecta--A case study from the Ries crater, southern Germany Item Type Article; text Authors Buchner, E.; Schmieder, M. Citation Buchner, E., & Schmieder, M. (2009). Multiple fluvial reworking of impact ejecta—A case study from the Ries crater, southern Germany. Meteoritics & Planetary Science, 44(7), 1051-1060. DOI 10.1111/j.1945-5100.2009.tb00787.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 06/10/2021 20:56:07 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656594 Meteoritics & Planetary Science 44, Nr 7, 1051–1060 (2009) Abstract available online at http://meteoritics.org Multiple fluvial reworking of impact ejecta—A case study from the Ries crater, southern Germany Elmar BUCHNER* and Martin SCHMIEDER Institut für Planetologie, Universität Stuttgart, 70174 Stuttgart, Germany *Corresponding author. E-mail: [email protected] (Received 21 July 2008; revision accepted 12 May 2009) Abstract–Impact ejecta eroded and transported by gravity flows, tsunamis, or glaciers have been reported from a number of impact structures on Earth. Impact ejecta reworked by fluvial processes, however, are sparsely mentioned in the literature. This suggests that shocked mineral grains and impact glasses are unstable when eroded and transported in a fluvial system. As a case study, we here present a report of impact ejecta affected by multiple fluvial reworking including rounded quartz grains with planar deformation features and diaplectic quartz and feldspar glass in pebbles of fluvial sandstones from the “Monheimer Höhensande” ~10 km east of the Ries crater in southern Germany. -
The Chiemgau Crater Strewn Field: Evidence of a Holocene Large Impact Event in Southeast Bavaria, Germany
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/259471241 The Chiemgau Crater Strewn Field: Evidence of a Holocene Large Impact Event in Southeast Bavaria, Germany Article · January 2010 CITATIONS READS 20 115 7 authors, including: Kord Ernstson Andreas Neumair University of Wuerzburg University of Salzburg 97 PUBLICATIONS 571 CITATIONS 33 PUBLICATIONS 102 CITATIONS SEE PROFILE SEE PROFILE Barbara Rappenglueck Michael A. Rappenglück Institute for Interdisciplinary Science, Gilching vhs Gilching and Observatory Gilching 16 PUBLICATIONS 72 CITATIONS 60 PUBLICATIONS 156 CITATIONS SEE PROFILE SEE PROFILE Some of the authors of this publication are also working on these related projects: The Digital Terrain Model (DTM) for the evaluation of Holocene meteorite craters. View project New approach to an old debate: The Pelarda Formation meteorite impact ejecta (Azuara structure, Iberian Chain, NE Spain) View project All content following this page was uploaded by Kord Ernstson on 28 December 2013. The user has requested enhancement of the downloaded file. Journal of Siberian Federal University. Engineering & Technologies 1 (2010 3) 72-103 ~ ~ ~ УДК 551.3 The Chiemgau Crater Strewn Field: Evidence of a Holocene Large Impact Event in Southeast Bavaria, Germany Kord Ernstson*a, Werner Mayerb, Andreas Neumairb, Barbara Rappenglückb, Michael A. Rappenglückb, Dirk Sudhausc and Kurt W. Zellerd a University of Würzburg, Am Judengarten 23, 97204 Höchberg, Germany b Institute for Interdisciplinary Studies, Bahnhofstraße 1, 82205 Gilching, Germany c Institute of Geography, University of Augsburg, Universitätsstraße 10, 86135 Augsburg, Germany d Österreichisches Forschungszentrum Dürrnberg, Pflegerplatz 5, 5400 Hallein, Austria 1 Received 30.01.2009, received in revised form 27.02.2010, accepted 9.03.2010 The Chiemgau strewn field in the Alpine Foreland discovered in the early new millennium comprises more than 80 mostly rimmed craters in a roughly elliptically shaped area with axes of about 60 km and 30 km. -
A New Way to Confirm Meteorite Impact Produced Planar Features in Quartz: Combining Universal Stage and Electron Backscatter Diffraction Techniques
A new way to confirm meteorite impact produced planar features in quartz: combining Universal Stage and Electron Backscatter Diffraction techniques M.H. Voorn MSc Thesis August 2010 Utrecht University - Earth Sciences department Structural Geology and Tectonic research group Abstract As recognised from the geological record, meteorite impact events can have a severe influence on (local) geology, climate and life. Solid evidence for these events is therefore important to obtain. The most convincing evidence comes from microstructures in quartz. Upon impact, Planar Fractures (PFs) and Planar Deformation Features (PDFs) form parallel to specific crystallographic planes in quartz. Non-impact formed (tectonic) Deformation Lamellae (DL) may be hard to distinguish qualitatively from PFs or PDFs with the optical microscope, but do not form parallel to crystallographic planes. Quantitative methods using the Universal Stage (U-Stage) on the optical microscope have therefore been applied widely to (dis)confirm this parallelism. With the method, the quartz c-axis and poles to planar features are measured and plotted. An improved technique requires so-called indexing of the measured orientations using a stereographic projection template. Even when these techniques are applied, some proposed impact structures remain debated. An important reason for this is the U-stage can not provide the full crystal orientation of quartz. The goal of this thesis was to check the classical U-stage techniques for quantitatively confirming impact planar features in quartz, and to see whether the addition of Electron Backscatter Diffraction (EBSD, on the Scanning Electron Microscope: SEM) and Cathodoluminescence (CL, on the SEM) can provide more solid evidence. Six previously confirmed impact and three non-impact samples were studied. -
Family Model 4
Is the South so different? Italian and Spanish Families in a Comparative Perspective Teresa Jurado Guerrero and Manuela Naldini Article published in South European Society and Politics, 1996, 1:3, pages 42 – 66. Summary: This article analyses family changes in Italy and Spain from 1960 to 1990 and contrasts them with four Central/Northern European countries. Italy and Spain show extremely rapid family changes, which nevertheless do not lead to a convergence between southern and cen- tral/northern families. The particularities of the southern family model are a high degree of cross-generational cohabitation, a high frequency of social contacts and help within kinship, a strong institutionalization of marriage, a low female employment rate in the formal labour market, a low fertility rate, and widespread family and child-oriented attitudes. In addition, relations between generations are seen more in terms of obligations than in terms of individ- ual choice. We conclude that the specific economic situation, the particularities of social poli- cies and the family culture in Italy and Spain are important barriers for a further individuali- zation of family relations in these societies. The aim of this paper is to analyse Italy and Spain as representatives of a Mediterranean type of society.1 The question whether such a type exists with respect to family changes will be explored here. For this purpose we use a comparative perspective. Our assumption is that the division of labour between state, family, labour market and church in Mediterranean countries is a specific one. The societal configuration in the South will be analysed from the perspective of the family. -
ANIC IMPACTS: MS and IRONMENTAL P ONS Abstracts Edited by Rainer Gersonde and Alexander Deutsch
ANIC IMPACTS: MS AND IRONMENTAL P ONS APRIL 15 - APRIL 17, 1999 Alfred Wegener Institute for Polar and Marine Research Bremerhaven, Germany Abstracts Edited by Rainer Gersonde and Alexander Deutsch Ber. Polarforsch. 343 (1999) ISSN 01 76 - 5027 Preface .......3 Acknowledgements .......6 Program ....... 7 Abstracts P. Agrinier, A. Deutsch, U. Schäre and I. Martinez: On the kinetics of reaction of CO, with hot Ca0 during impact events: An experimental study. .11 L. Ainsaar and M. Semidor: Long-term effect of the Kärdl impact crater (Hiiumaa, Estonia) On the middle Ordovician carbonate sedimentation. ......13 N. Artemieva and V.Shuvalov: Shock zones on the ocean floor - Numerical simulations. ......16 H. Bahlburg and P. Claeys: Tsunami deposit or not: The problem of interpreting the siliciclastic K/T sections in northeastern Mexico. ......19 R. Coccioni, D. Basso, H. Brinkhuis, S. Galeotti, S. Gardin, S. Monechi, E. Morettini, M. Renard, S. Spezzaferri, and M. van der Hoeven: Environmental perturbation following a late Eocene impact event: Evidence from the Massignano Section, Italy. ......21 I von Dalwigk and J. Ormö Formation of resurge gullies at impacts at sea: the Lockne crater, Sweden. ......24 J. Ebbing, P. Janle, J, Koulouris and B. Milkereit: Palaeotopography of the Chicxulub impact crater and implications for oceanic craters. .25 V. Feldman and S.Kotelnikov: The methods of shock pressure estimation in impacted rocks. ......28 J.-A. Flores, F. J. Sierro and R. Gersonde: Calcareous plankton stratigraphies from the "Eltanin" asteroid impact area: Strategies for geological and paleoceanographic reconstruction. ......29 M.V.Gerasimov, Y. P. Dikov, 0 . I. Yakovlev and F.Wlotzka: Experimental investigation of the role of water in the impact vaporization chemistry. -
Ages of Large Lunar Impact Craters and Implications for Bombardment During the Moon’S Middle Age ⇑ Michelle R
Icarus 225 (2013) 325–341 Contents lists available at SciVerse ScienceDirect Icarus journal homepage: www.elsevier.com/locate/icarus Ages of large lunar impact craters and implications for bombardment during the Moon’s middle age ⇑ Michelle R. Kirchoff , Clark R. Chapman, Simone Marchi, Kristen M. Curtis, Brian Enke, William F. Bottke Southwest Research Institute, 1050 Walnut Street, Suite 300, Boulder, CO 80302, United States article info abstract Article history: Standard lunar chronologies, based on combining lunar sample radiometric ages with impact crater den- Received 20 October 2012 sities of inferred associated units, have lately been questioned about the robustness of their interpreta- Revised 28 February 2013 tions of the temporal dependance of the lunar impact flux. In particular, there has been increasing focus Accepted 10 March 2013 on the ‘‘middle age’’ of lunar bombardment, from the end of the Late Heavy Bombardment (3.8 Ga) until Available online 1 April 2013 comparatively recent times (1 Ga). To gain a better understanding of impact flux in this time period, we determined and analyzed the cratering ages of selected terrains on the Moon. We required distinct ter- Keywords: rains with random locations and areas large enough to achieve good statistics for the small, superposed Moon, Surface crater size–frequency distributions to be compiled. Therefore, we selected 40 lunar craters with diameter Cratering Impact processes 90 km and determined the model ages of their floors by measuring the density of superposed craters using the Lunar Reconnaissance Orbiter Wide Angle Camera mosaic. Absolute model ages were computed using the Model Production Function of Marchi et al. -
The Subsurface Structure of Oblique Impact Craters
The subsurface structure of oblique impact craters Dissertation vorgelegt von Dipl.-Geol. Michael H. Poelchau vom Fachbereich Geowissenschaften der Freien Universität Berlin zur Erlangung des akademischen Grades doctor rerum naturalium (Dr. rer. nat.) Berlin, 2010 The subsurface structure of oblique impact craters Dissertation vorgelegt von Dipl.-Geol. Michael H. Poelchau vom Fachbereich Geowissenschaften der Freien Universität Berlin zur Erlangung des akademischen Grades doctor rerum naturalium (Dr. rer. nat.) Berlin, 2010 Gutachter: 1. PD Dr. Thomas Kenkmann 2. Prof. Wolf-Uwe Reimold Tag der Disputation: 23.02.2010 Statement regarding the contributions of the author and others to this thesis This thesis is comprised of three published, peer-reviewed articles and one submitted manuscript, which each form separate chapters within this thesis. The chapters “Introduction” and “General Conclusions” were written especially for this thesis. The PhD candidate is the first author of two of these articles, and the second author of the third article. The PhD candidate is also the first author of a manuscript currently submitted to Earth and Planetary Science Letters. Therefore, these four chapters have their own introduction, methodology, discussion, conclusions and references. The articles and manuscripts used in this thesis are the following: Poelchau, M. H., and T. Kenkmann, 2008. Asymmetric signatures in simple craters as an indicator for an oblique impact direction, Meteoritcal and Planetary Science, 43, 2059-2072. Poelchau M. H., Kenkmann T. and Kring D. A., 2009. Rim uplift and crater shape in Meteor Crater: the effects of target heterogeneities and trajectory obliquity. Journal of Geophysical Research, 114, E01006, doi:10.1029/2008JE003235. Kenkmann, T.